She is also quoted as saying (similar to what you said above) , that the object will eventually completely sublimate.
My understanding so far was that once all the volatiles are gone comets will essentially resemble asteroids (i.e. extinct comets). Maybe this would be only true for some comets?
Or she was not being precise enough -- the rocky parts of comets won't sublimate.
BTW, in another messageboard, someone claimed that the enrichment of a certain dust grain in sodium was due to sublimation. The original results:
COSIMA detects sodium and magnesium in a dust grain called Boris | Rosetta - ESA's comet chaser COSIMA measured Na-23+ and Mg-24+ and found
(Na)/(Mg) peak heights = 4.6
This is unusual enrichment in sodium by Solar-System standards.
The bulk composition of rocky materials in the Solar System, as far as it can be inferred, is mafic or basaltic, enriched in magnesium and iron. In the Sun and some meteorites,
(Na)/(Mg) atoms = 0.05 - 0.06
The Earth's continental crust is enriched in sodium because of fractionation of magmas, making it felsic or granitic.
(Na)/(Mg) atoms = 0.75 to 2.0 (estimates jump around quite a bit)
But Boris is even more enriched in sodium.
This cannot be due to sublimation at 67P's getting as close as it does to the Sun, because rocky materials are generally very refractory. One would have to go *very* close the Sun to make them start to boil off.
So this grain either formed when the Solar System formed or else was a grain from some other star that found its way into the protosolar nebula.
The Rosetta team ought to look for more elements, and also analyze more grains, but they might only release their results when they are ready to publish them.